Radiation Backreaction in Spinning Binaries
| dc.creator | Gergely, László Á. | |
| dc.creator | Perjés, Zoltán | |
| dc.creator | Vasúth, Mátyás | |
| dc.date | 1998-01-02 | |
| dc.date.accessioned | 2026-07-07T03:32:08Z | |
| dc.date.available | 2026-07-07T03:32:08Z | |
| dc.description | The evolution under radiation backreaction of a binary system consisting of a black hole and a companion is studied in the limiting case when the spin of the companion is negligible compared with the spin S of the black hole. To first order in the spin, the motion of the reduced-mass particle excluding radiation effects, is characterized by three constants: the energy E, the magnitude L of the angular momentum and the projection L_S of the angular momentum along the spin S. This motion is quasiperiodic with a period determined by r_{min} and r_{max}. We introduce a new parametrization, making the integration over a period of a generic orbit especially simple. We give the averaged losses in terms of the 'constants of motion' during one period for generic orbits, to linear order in spin. | |
| dc.description | 3 pages, to appear in the Proceedings of the 8th Marcel Grossmann Meeting | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9801002 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9801002 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/36115 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Radiation Backreaction in Spinning Binaries | |
| dc.type | text |